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<category>Cosmology and Particle Astrophysics</category>
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<announcer>
 <user>
  <title>Prof.</title>
  <name first="Karl-Heinz" middle="" last="Kampert"></name>
  <organization>Bergische Universitaet Wuppertal (DE)</organization>
  <email>karl-heinz.kampert@cern.ch</email>
  <userid>42616</userid>
 </user>
</announcer>
<supportEmail caption="Contact">conf@2012.uhecr.org</supportEmail>
<title>International Symposium on Future Directions in UHECR Physics</title>
<description>This Workshop is the follow-up of the &lt;a href="http://uhecr2010.icrr.u-tokyo.ac.jp/"&gt;Nagoya Symposium 2010&lt;/a&gt;&lt;br /&gt;
&lt;br /&gt;
&lt;strong&gt;Scope of the Workhop:&lt;/strong&gt;&lt;br /&gt;
&lt;ul&gt;
	&lt;li&gt;
		Discuss the highlights and challenges of UHECR observations&lt;/li&gt;
	&lt;li&gt;
		Prepare for a next-generation ground based giant detector&lt;/li&gt;
	&lt;li&gt;
		Evaluate the complementarity of ground and space based observations&lt;/li&gt;
	&lt;li&gt;
		Identify technological challenges and related R&amp;amp;D works&lt;/li&gt;
&lt;/ul&gt;
</description>
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<closed>False</closed>
<location>
 <name>CERN</name>
 <address>CERN, Geneva</address>
 <room>500-1-001 - Main Auditorium</room>
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</location>
<startDate>2012-02-13T14:00:00</startDate>
<endDate>2012-02-16T18:00:00</endDate>
<creationDate>2011-08-22T11:17:56</creationDate>
<modificationDate>2012-04-07T08:03:12</modificationDate>
<timezone>Europe/Zurich</timezone>
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 <title>Hybrid analysis for the Telescope Array</title>
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   <title>Dr.</title>
   <name first="Daisuke" middle="" last="Ikeda"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <email>ikeda@icrr.u-tokyo.ac.jp</email>
  </user>
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 <primaryAuthors>
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   <title>Dr.</title>
   <name first="Daisuke" middle="" last="Ikeda"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <email>ikeda@icrr.u-tokyo.ac.jp</email>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title></title>
   <name first="Elliott" middle="" last="Barcikowski"></name>
   <organization>University of Utah</organization>
   <email>elliottb@cosmic.utah.edu</email>
  </user>
  <user>
   <title></title>
   <name first="Hiroyuki" middle="" last="Sagawa"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <email>hsagawa@icrr.u-tokyo.ac.jp</email>
  </user>
  <user>
   <title></title>
   <name first="Benjamin" middle="" last="Stokes"></name>
   <organization>University of Utah</organization>
   <email>stokes@cosmic.utah.edu</email>
  </user>
  <user>
   <title></title>
   <name first="Gordon" middle="" last="Thomson"></name>
   <organization>University of Utah</organization>
   <email>thomson@physics.utah.edu</email>
  </user>
  <user>
   <title></title>
   <name first="Tareq" middle="" last="Abu-Zayyad"></name>
   <organization>University of Utah</organization>
   <email>tareq@cosmic.utah.edu</email>
  </user>
  <user>
   <title></title>
   <name first="Monica" middle="" last="Allen"></name>
   <organization>University of Utah</organization>
   <email>monica@cosmic.utah.ed</email>
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 </coAuthors>
 <location>
  <name>CERN</name>
  <address>CERN, Geneva</address>
  <room>500-1-001 - Main Auditorium</room>
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 <abstract>The Telescope Array (TA) experiment is the largest Ultra-High Energy Cosmic Ray (UHECR) observatory in the northern hemisphere, and is located in the west desert of Utah. It is a hybrid UHECR experiment using two types of detectors: three stations of Fluorescence Detectors (FDs) and 507 Surface Detectors (SDs). The three FD stations (at Middle Drum (MD), Long Ridge (LR), and Black Rock (BR)) overlook the SD array. The MD station consists of 14 refurbished HiRes-I telescopes. The BR and LR stations are newly constructed for the TA experiment. The events detected by both SD and FD are reconstructed by the hybrid technique, which uses information from both the SD and FD. The resolution reaches &lt; 1 degree for arrival directions and &lt; 10% in energy. Hybrid events are used to compare the FD and SD energy scales, measure the spectrum, and determine the composition of cosmic rays. In this talk we present the performance of the hybrid technique for the BR, LR, and MD stations.</abstract>
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